Recent DESI DR1 and DR2 data indicate mild time evolution in the dark-energy equation of state, while persistent discrepancies between early- and late-universe probes continue to manifest as the Hubble tension (∆H0 ≈5−6 km/s/Mpc,∼4−5σ) and the S8 tension (∼2−3σ). We demonstrate that both tensions are naturally resolved within [a new]Framework by a single, minimal extension: a brief, entropy-driven early dark energy (EDE) phase triggered by Twin-Law charge buildup before recombination, followed by the late- time charge-discharge mechanism already derived in our prior work. The early EDE phase arises automatically when the Hubble friction term 3H|˙ϕ|drops below the fixed potential tilt ϵ, a crossover that occurs at the cosmologically natural temperature T ≈0.95 eV (z ≈ 3500) set entirely by the benchmark parameters of the scalar potential. A transient energy release fEDE ≈0.13−0.15 raises the CMB-inferredH0 from 67.4 to∼72.8 km/s/Mpc, while the subsequent late-time charge-discharge produces the mild phantom-like w(z) evolution pre-ferred by DESI. Full CLASS/CAMB Markov-chain Monte-Carlo fits to the combined Planck+ACT+DESI DR2+BAO+Pantheon++KiDS/HSC 1 dataset reduce the Hubble tension to < 2σ and the S8 tension to<1.5σ with only the original model parameters.The mechanism preserves all prior predictions, including a distinctive stochastic ravitational-wave background with a softened infrared tail and secondary mHz hump inside the LISA core band, as well as a specific w(z) wiggle observable in forthcoming DESI DR3/DR4 re-leases. The framework remains fully consistent with the Twin Laws of energy and information conservation and requires no fine-tuningbeyond the parameters already fixed in our earlier work. We discuss falsifiability and the string-theory UV completion via Bento—Monteroflux compactifications.